Since the discovery of the phenomenon of superconductivity in mercury by Heike Kammerlingh Onnes in 1911, the search for new compounds with higher transition temperatures has presented a continuous challenge in the field of materials science. After the discovery of the Nb <inf xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">3</inf> Sn superconductors with A 15-type structure, the efforts, mainly concentrated on intermetallic compounds, experienced steady but slow success. With a T <inf xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">c</inf> of 23.3 K in Nb <inf xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">3</inf> Ge, however, a limit seemed to have been approached. Reports of materials with higher T <inf xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">c</inf> appeared occasionally, but these could not withstand the critical tests. Superconductivity research was just celebrating its 75th anniversary in 1986, when interest in the field was sparked by the discovery of a new class of metallic perovskite-type copper-based oxides with transition temperatures of 35 K.
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